most citedThe fast filament eruption leading to the X-flare on March 29, 2014

63 citations · 208 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201737 cited

A Statistical Study of Photospheric Magnetic Field Changes During 75 Solar Flares

J. S. Castellanos Durán, L. Kleint, B. Calvo-Mozo

Abrupt and permanent changes of photospheric magnetic fields have been observed during solar flares. The changes seem to be linked to the reconfiguration of magnetic fields, but th…

astro-ph.SR2017

Measurement of the evolution of the magnetic field of the quiet photosphere during a solar cycle

Renzo Ramelli, Michele Bianda, Svetlana Berdyugina +2

The solar photosphere is filled by a magnetic field which is tangled on scales much smaller than the resolution capability of solar telescopes. This hidden magnetic field can be in…

astro-ph.SR201738 cited

On the nature of off-limb flare continuum sources detected by SDO/HMI

P. Heinzel, L. Kleint, J. Kasparova +1

The Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory has provided unique observations of off-limb flare emission. White-light (WL) continuum enhancements wer…

astro-ph.SR201722 cited

On the origin of the flare emission in IRIS' SJI 2832 filter: Balmer continuum or spectral lines?

Lucia Kleint, Petr Heinzel, Säm Krucker

Continuum ("White-light", WL) emission dominates the energetics of flares. Filter-based observations, such as the IRIS SJI 2832 filter, show WL-like brightenings during flares, but…

astro-ph.SR201563 cited

The fast filament eruption leading to the X-flare on March 29, 2014

Lucia Kleint, Marina Battaglia, Kevin Reardon +3

We investigate the sequence of events leading to the solar X1 flare SOL2014-03-29T17:48. Because of the unprecedented joint observations of an X-flare with the ground-based Dunn So…

astro-ph.SR201548 cited

Internetwork chromospheric bright grains observed with IRIS

Juan Martínez-Sykora, Luc Rouppe van der Voort, Mats Carlsson +18

The Interface Region Imaging Spectrograph (IRIS) reveals small-scale rapid brightenings in the form of bright grains all over coronal holes and the quiet sun. These bright grains a…